Algol As Horus in the Cairo Calendar 233 Radius Than Algol A
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Open Astron. 2018; 27: 232–264 Research Article Sebastian Porceddu*, Lauri Jetsu, Tapio Markkanen, Joonas Lyytinen, Perttu Kajatkari, Jyri Lehtinen, and Jaana Toivari-Viitala Algol as Horus in the Cairo Calendar: the possible means and the motives of the observations https://doi.org/10.1515/astro-2018-0033 Received Feb 15, 2018; accepted May 04, 2018 Abstract: An ancient Egyptian Calendar of Lucky and Unlucky Days, the Cairo Calendar (CC), assigns luck with the period of 2.850 days. Previous astronomical, astrophysical and statistical analyses of CC support the idea that this was the period of the eclipsing binary Algol three millennia ago. However, next to nothing is known about who recorded Algol’s period into CC and especially how. Here, we show that the ancient Egyptian scribes had the possible means and the motives for such astronomical observations. Their principles of describing celestial phenomena as activity of gods reveal why Algol received the title of Horus Keywords: Algol, Horus, ancient Egyptian Astronomy, variable stars, the Cairo Calendar, hemerologies 1 Introduction dated to 1271-1163 B.C. (Bakir 1966, p2-5), (Van Walsem 1982, p233) and (Helck et al. 1975–1992, p156), and pub- lished by Abd el-Mohsen Bakir. As in all our three pre- The ancient Egyptian texts known as the Calendars of vious studies (Porceddu et al. 2008; Jetsu et al. 2013; Lucky and Unlucky Days, or hemerologies, are literary Jetsu and Porceddu 2015), we use only the best preserved works that assign prognoses to each day of the Egyptian continuous calendar which is found on pages recto III- year (Wells 2001a, p117-118), (Leitz 1994, p1-2) (Bacs XXX and verso I-IX of papyrus Cairo 86637. The other 1990, p41-45) (Troy 1989, p127-147) and (Helck et al. texts and fragments contained in the same papyrus are ig- 1975–1992, p156). These prognoses denote whether the nored from this analysis because the connection of these day, or a part of the day, is considered “good”Nor “bad”N. fragments to the main calendar is not apparent and we 1 Nine such texts have been found (Troy 1989, p140-143), do not know what year they describe, so combining any (Leitz 1994, p-2) and (Porceddu et al. 2008, p328). Here, data points from these sources to the dataset created from we study the best preserved one of these nine texts, CC, the long Cairo Calendar would introduce a random noise component to the analysis. All CC text passages we quote Corresponding Author: Sebastian Porceddu: Department in this article have been translated by us from the hi- of Physics, University of Helsinki, Finland; eroglyphic transcription of Leitz (1994), assisted by the Email: sebastian.porceddu@helsinki.fi translations of Bakir (1966, in English) and Leitz (1994, Lauri Jetsu: Department of Physics, University of Helsinki, Fin- arXiv:1810.06412v1 [physics.hist-ph] 5 Oct 2018 in German). land The synodic period of the Moon was discovered in CC Tapio Markkanen: Department of Physics, University of Helsinki, Finland with a statistical method called the Rayleigh test, as well Joonas Lyytinen: Department of Physics, University of Helsinki, as a few other periods (Porceddu et al. 2008, p334). In a Finland footnote of that study, it was noted that one seemingly Perttu Kajatkari: Department of Physics, University of Helsinki, less significant period, 2.850 days, was rather close to the Finland current 2.867 days period of Algol (β Persei). This star Jyri Lehtinen: Max-Planck-Institut für Sonnensystemforschung, is a prototype of a class of stars called eclipsing binaries. Göttingen, Germany Jaana Toivari-Viitala: Department of World Cultures, Univer- The two stars, Algol A and Algol B, orbit around a com- sity of Helsinki, Finland mon centre of mass with a period of 2.867 days. Algol A 1 We use the symbol “N” to denote the words and phrases trans- is brighter than Algol B. However, Algol B has a larger lated into Ancient Egyptian language in the list of Appendix A. Open Access. © 2018 S. Porceddu et al., published by De Gruyter. This work is licensed under the Creative Commons Attribution-NonCommercial- NoDerivatives 4.0 License S. Porceddu et al., Algol as Horus in the Cairo Calendar 233 radius than Algol A. Our line of sight nearly coincides (1783) determined the 2.867 days period of Algol in 1783. with the orbital plane of this double star system. There- A close friend and tutor of John Goodricke, Edward Pig- fore, these stars eclipse each other during every orbital ott, also discovered several new variable stars (Hoskin round. In a primary eclipse, the dimmer Algol B partly 1979). In his last paper, Pigott (1805, p152) argued that eclipses the brighter Algol A. This primary eclipse can the brightness of Algol must have been constant in An- be observed with naked eye. In a secondary eclipse, the tiquity, because the variability that he observed was so brighter Algol A partly eclipses the dimmer Algol B, but easy to notice with naked eyes. Kopal (1946, p3) sug- the decrease in total brightness of this binary system is gested that those ancient discoveries “may have been so small that this secondary eclipse event can not be ob- buried in the ashes of the Library of Alexandria”. More re- served with naked eye. Hence, the brightness of Algol ap- cently, Wilk (2000) has presented the theory that classical pears to remain constant for a naked eye observer, except mythology contains knowledge of the variability of vari- during the primary eclipses. These primary eclipses last ous stars, including Algol. This star also seems to belong about ten hours. For most of the time, Algol is brighter to the constellation called “Elk” by the Siberian shamans than its six close-by bright comparison stars (Jetsu et al. of the Khanty tribe, who have noticed that this animal 2013, their Figure 5a). During a primary eclipse, Algol sometimes loses one pair of legs (Pentikäinen 1997, p58- first becomes dimmer for five hours and then regains its 65). brightness in another five hours. For a few hours, Algol A statistical analysis of 28 selected words (hereafter appears visibly dimmer than all its six comparison stars. SWs) of the mythological narratives of CC was performed A naked eye observer can easily notice this as a clear to find traces of the Egyptians’ symbolism for Algol (Jetsu change in Algol’s constellation pattern. and Porceddu 2015). We notate the SWs of that par- The normalized Rayleigh test of the CC data con- ticular study for example “Horus” or “Seth” to distin- firmed the high significance of the 2.850 days period guish them from other Egyptian deities such as Isis and (Jetsu et al. 2013). The period increase from 2.850 to Nephthys. Out of all 28 SWs, the word “Horus” had the 2.867 days during the past three millennia gave a mass strongest connection to the 2.850 days periodicity (Jetsu transfer rate estimate from Algol B to Algol A. This esti- and Porceddu 2015). “Horus”, etymologically “the distant mate of Jetsu et al. (2013) agreed with the one predicted one”, was one of the earliest attested Egyptian deities. by the best evolutionary model of Algol (Sarna 1993, Predominantly a sky god or stellar god, the living king p540). A sequence of eight astronomical criteria was also was identified as an earthly “Horus” (Roeder 1994, p42- presented which proved that the ancient Egyptians could 43) and (Meltzer 2001, p119-122). Horus is described as a have discovered Algol’s periodic variability with naked star in the oldest ancient Egyptian texts (Krauss 2016). eyes (Jetsu et al. 2013, p9-10), i.e. it is the star where it Another deity, “Seth”, the adversary of “Horus”, was is easiest to discover regular short-term variability with- shown to be connected to the period of the Moon (Jetsu out the aid of a telescope. and Porceddu 2015). In the Hellenistic tradition, Algol was called “the Statistical analyses have confirmed the ancient Egyp- head of Gorgon”. Similar tradition was continued in the tian discovery of Algol’s period (Porceddu et al. 2008; Arabic name “Demon’s Head”. The name Algol is derived Jetsu et al. 2013; Jetsu and Porceddu 2015). Here, our from the Arabic word, head of the Ghoul (ra’s al-gh¯ul) aim is to connect this astonishing ancient discovery to its (Davis 1957). These names seem to indicate that some contemporary cultural and historical background by pre- exotic or foreboding feature or mutability was known in senting ten general arguments about CC (Sects 4.1-4.10). the folklore of the ancient peoples. All the way to me- These arguments strongly support the idea that the an- dieval astrology, the ill omens associated with the “evil cient Egyptian scribes had the possible means and the eye” of Algol were known, so it is actually surprising that motives to record Algol’s period into CC. The connection it is so difficult to find any direct reference to Algol’s vari- of CC mythological texts to the perceived behaviour of ability in old astronomical texts (Davis 1957). The list of the Moon and Algol is verified in Sects 4.7 and 4.8. ill-omened names is so impressive (Allen 1899, p332-333) that it is unlikely that the variability would have gone undetected through millennia of practical star observing by the ancient Egyptians. Of the modern astronomers, Fabricius discovered the first variable star, Mira, in 1596. The second variable star, Algol, was discovered by Montanari in 1669. Goodricke 234 S. Porceddu et al., Algol as Horus in the Cairo Calendar 2 2 Materials and Methods 1) .